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Breaking the Speed Limit: High-Speed Optical Coherence Modulation With Lithium Niobate

Overcoming conventional technological limitations to realize high-speed optical coherence modulation at 350 kHz. Structured light fields possess a wide range of unique and powerful characteristics. By gaining greater control over their optical coherence, researchers can not only reduce the drawba

Simulating the Hawking effect and other quantum field theory predictions with polariton fluids

Quantum field theory (QFT) is a physics framework that describes how particles and forces behave based on principles rooted in quantum mechanics and Albert Einstein’s special relativity theory. This framework predicts the emergence of various remarkable effects in curved spacetimes, including Hawking radiation.

Hawking radiation is the thermal radiation theorized to be emitted by close to the (i.e., the boundary around a black hole after which gravity becomes too strong for anything to escape). As ascertaining the existence of Hawking radiation and testing other QFT predictions in space is currently impossible, physicists have been trying to identify that could mimic aspects of curved spacetimes in experimental settings.

Researchers at Sorbonne University recently identified a new promising experimental platform for simulating QFT and testing its predictions. Their proposed QFT simulator, outlined in a paper published in Physical Review Letters, consists of a one-dimensional quantum fluid made of polaritons, quasiparticles that emerge from strong interactions between photons (i.e., light particles) and excitons (i.e., bound pairs of electrons and holes in semiconductors).

This ‘super-Earth’ exoplanet 35 light-years away might have what it takes to support life

“Finding a temperate planet in such a compact system makes this discovery particularly exciting,” Charles Cadieux, a postdoctoral researcher at the university and lead author of the study, said in the statement. “It highlights the remarkable diversity of exoplanetary systems and strengthens the case for studying potentially habitable worlds around low-mass stars.”

L 98–59 f was discovered by reanalyzing data from the European Southern Observatory’s (ESO) HARPS (High Accuracy Radial velocity Planet Searcher) and ESPRESSO (Echelle Spectrograph for Rocky Exoplanet and Stable Spectroscopic Observations) spectrographs. Since the exoplanet doesn’t transit, or pass in front of, its host star from our perspective, astronomers spotted it by tracking subtle shifts in the star’s motion that are caused by the planet’s gravitational pull.

By combining the spectrograph data with observations from NASA’s TESS (Transiting Exoplanet Survey Satellite) and James Webb Space Telescope (JWST) — and using advanced techniques to filter out stellar noise — researchers were able to determine the size, mass and key properties of all five planets.

Study offers clearer picture of childhood brain tumor survival

Childhood brain tumor survival depends on the type of tumor. Comparing survival rates across countries is difficult, because brain tumors aren’t recorded in the same way everywhere in Europe. A new study led by the Princess Máxima Center is helping to change that. For the first time, the research provides a clear and clinically relevant overview of survival outcomes for children with brain tumors.

Researchers at the Princess Máxima Center analyzed data from more than 30,000 diagnosed with a brain tumor between 1998 and 2013. The data came from 80 cancer registries across 31 European countries. The study was published today in The Lancet Oncology.